Isostatic and dynamic support of high topography

Earth and Planetary Science Letters 446 (2016) 1–9
Contents lists available at ScienceDirect
Earth and Planetary Science Letters
www.elsevier.com/locate/epsl
Isostatic and dynamic support of high topography on a North Atlantic
passive margin
Vivi K. Pedersen a,∗ , Ritske S. Huismans a , Robert Moucha b
a
b
Department of Earth Science, University of Bergen, Allegaten 41, N-5007 Bergen, Norway
Department of Earth Sciences, Syracuse University, Syracuse, NY 13210, United States
a r t i c l e
i n f o
Article history:
Received 9 October 2015
Received in revised form 18 April 2016
Accepted 19 April 2016
Available online xxxx
Editor: A. Yin
Keywords:
isostasy
dynamic topography
passive margin topography
Scandinavia
a b s t r a c t
Substantial controversy surrounds the origin of high topography along passive continental margins. Here
we focus on the well-documented elevated passive margin in southwestern Scandinavia, and quantify the
relative contributions of crustal isostasy and dynamic topography in controlling the present topography.
We find that majority of the topography is compensated by the crustal structure, suggesting a topographic
age that is in accord with the 400 Myr old Caledonian orogenesis. In addition, we propose that dynamic
uplift of ∼300 m has rejuvenated existing topography locally in the coastal region over the last 10 Myr.
Such uplift, combined with a general sea level fall, can help explain a variety of observations that have
traditionally been interpreted in favor of a peneplain uplift model. We conclude that high topography
along the Scandinavian margin cannot represent remnants of a peneplain uplifted within the last 20 Myr.
The topography must have been high since the Caledonian orogeny.
© 2016 Elsevier B.V. All rights reserved.
1. Introduction
A surprisingly significant part of global high topography is associated with rifted passive continental margins such as along the
North Atlantic margins in Scandinavia and Greenland, the south
Atlantic Brazilian and African margins, the east Australian margin, the Red Sea, and western India. A number of mechanisms
have been suggested for such high topography to exist far beyond the most recent period of active rifting, including flexural
isostasy related to i) lithosphere necking (Braun and Beaumont,
1989), ii) mechanical unloading during extension (Weissel and
Karner, 1989), and iii) differential denudation (Gilchrist and Summerfield, 1990). Other mechanisms include underplating and intrusions in the lower crust (McKenzie, 1984), anticlinal, lithospheric
folds caused by compression (Japsen et al., 2012), and the notion
that topography may have survived orogenic collapse and rifting to
leave again remnants from earlier orogenesis (Nielsen et al., 2009).
However, a comprehensive understanding of why these margins
are elevated today and whether they share a common origin remains enigmatic. Herein we focus on the well-documented southwestern Scandinavian margin in the North Atlantic as an archetype
of an elevated passive continental margin.
*
Corresponding author.
E-mail address: [email protected] (V.K. Pedersen).
http://dx.doi.org/10.1016/j.epsl.2016.04.019
0012-821X/© 2016 Elsevier B.V. All rights reserved.
The topography in western Scandinavia shows distinct highelevation low-relief regions that have traditionally been interpreted
as remnants of a Mesozoic peneplain uplifted in the Cenozoic
(Fig. 1, Hypothesis 1, time frame T2–T3; e.g. Lidmar-Bergström
et al., 2000). This interpretation has been supported by offshore
studies identifying increased sedimentation in the Cenozoic, overburial of coast-proximal tilted sedimentary strata, and an angular
unconformity at the base of the Quaternary (e.g. Japsen, 1988;
Riis, 1996; Stuevold and Eldholm, 1996). However, it has also
been recently suggested that prolonged climate-dependent erosion
and isostatic uplift of old remnant topography from the Caledonian orogeny that survived Mesozoic and early Cenozoic rifting may equally well explain these key observations (Fig. 1, Hypothesis 2, T1–T3; Goledowski et al., 2012; Nielsen et al., 2009;
Steer et al., 2012).
These diametrically opposing end-member hypotheses imply
distinctly different crustal structure and degree of crustal compensation of present-day topography (Fig. 1). Peneplain formation
requires complete erosion of existing topography to the degree
where any crustal root has been obliterated. The peneplain in Hypothesis 1 should therefore be associated with a non-buoyant crust
(Fig. 1, T2). This should also be the case for an uplifted peneplain
(Fig. 1, T3). For the inherited remnant topography in Hypothesis 2,
a thickened buoyant crust is expected to compensate all presentday topography (Fig. 1, T2–T3). We emphasize in this context, that
a thin crust may compensate positive topography, if low-density
material acts as a crustal root (mass deficit). Conversely, a thick
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V.K. Pedersen et al. / Earth and Planetary Science Letters 446 (2016) 1–9
Here we quantify the degree of isostatic topographic compensation using refraction seismic data (Stratford et al., 2009) to
constrain a hybrid approach considering crustal thickness (Airy
isostasy), crustal density (Pratt isostasy), and the flexural strength
of the lithosphere. We combine these quantitative estimates with
predictions of recent dynamic uplift in order to test whether a
combination of elements from previous end-member hypotheses
may best explain the current high topography along this margin
(Fig. 1, Hypothesis 3).
2. Methods
2.1. Local isostatic compensation of topography
We compute the degree of local isostatic compensation of
present-day topography by the crustal structure with a threedimensional density structure based on recently published seismic
data from southern Norway (Stratford et al., 2009). These new
seismic observations permit us to define a general velocity–depth
relationship for this region by assuming a linear increase in velocity between four tie-points down through the crust (Fig. 3B). We
convert this velocity model to density using a standard procedure
described in Brocher (2005).
We calculate the amount of topography that can be compensated locally by the crust by balancing the load of each crustal
column against a reference crustal column down to a common
compensation depth where no lateral variation in density is assumed. That is,
moho
ρtopo hisostasy g +
ρcrust (z) g dz =
0
Fig. 1. Schematic models for post-Caledonian geodynamic evolution in western
Scandinavia. Existing hypotheses (Hypothesis 1 and Hypothesis 2) for the geodynamic evolution of western Scandinavia since the Caledonian orogeny illustrated
by crust and topography structure at three snapshots in time (T1, T2, T3), and
the hypothesis proposed in this study (Hypothesis 3). Dashed black lines represent
a reference crustal thickness with zero compensated topography. Arrows indicate
changes in surface elevation. Note figure is not to scale.
crust cannot necessarily compensate significant positive topography, if the buoyancy-effect of the crustal root is reduced by highdensity material (mass excess).
The high topography along the Scandinavian margin roughly coincides with a significant negative (∼ −85 mGal) Bouguer gravity
anomaly (Fig. 2; Balling, 1980; Pavlis et al., 2012) and suggests
that a mass deficit exists at depth. The relatively short wavelength of the gravity anomaly (∼250 km) compared to crust- and
lithosphere-thickness indicates that this mass deficit is located at
shallow crustal depths and may compensate part or all of the
present-day topography. However, the degree of compensation by
the crustal structure is still debated, in part because an offset
exists between the maximum topography and the thickest crust,
and because of possible contributions from the lithospheric mantle
and/or the asthenosphere (Ebbing and Olesen, 2005; Ebbing, 2007;
Ebbing et al., 2012; England and Ebbing, 2012; Maupin et al., 2013;
Stratford et al., 2009).
Cref
ρCref (z) g dz + ρm rg
0
where on the left-hand-side, the load of any local crustal column
is given by the sum of the topographic load and the load of the
crust. We assume a constant topographic load density ρtopo of
2670 kg/m3 , corresponding to observed P-wave velocities at sea
level. The crustal load is found by integrating the depth-dependent
density profile ρcrust ( z) from sea level down to the local Moho
depth. On the right-hand-side, the reference column is defined
as the load of a reference crust with thickness Cref and depthdependent density profile, ρCref ( z), plus a load from the mantle
corresponding to any excess crust at the specific location (r =
moho − Cref ). The mantle lithosphere density ρm is assumed constant (3300 kg/m3 ). With this load balance we can determine the
local isostatically compensated topography hisostasy :
Cref
hisostasy =
0
ρCref (z)dz + ρm r −
ρtopo
moho
0
ρcrust (z)dz
.
For regions where the estimated isostatically compensated topography is less than zero, we substitute hisostasy with a corrected water depth d. The correction is done using the local depth-averaged
crustal density, ρavc , iterating in order to consider the effect of
the water depth, d, on the averaged crustal density itself, and the
change in Moho thickness due to the water load.
d = a
(ρm − ρavc )
(ρavc − ρ w )
where a is the thickness of the crustal deficit (a = −r) and
ρ w is the density of water.
The topography that can be locally compensated by a given
crustal structure will depend on the choice of a reference crustal
column that is assumed to give rise to zero topography. This is,
however, inherently difficult to determine, because part of the topography may be due to buoyancy effects from within the mantle
V.K. Pedersen et al. / Earth and Planetary Science Letters 446 (2016) 1–9
3
Fig. 2. Observations in Scandinavia. A. Colors indicate topography and bathymetry, whereas contour lines represent depth to the seismic Moho in km (Stratford et al., 2009).
B. Colors represent Bouguer anomaly (http://bgi.omp.obs-mip.fr/; Fuella et al., 2008; Pavlis et al., 2012), whereas contours represent the effective elastic thickness in km
(Pérez-Gussinyé and Watt, 2005). C. Colors represent free-air gravity anomaly (http://bgi.omp.obs-mip.fr/; Fuella et al., 2008; Pavlis et al., 2012).
Fig. 3. Topography, density and gravity anomaly across southwestern Scandinavia. A. Elevation along transect (for location see Fig. 1). B. Density with depth along transect.
Two vertical seismic velocity profiles illustrate the 4-point velocity model used to generate the density model. LCB indicates lower crustal body (see text). The reference
crustal column is shown to the right. C. Density anomaly along transect with respect to reference crust (see B) and the resulting Bouguer gravity anomaly (red line)
compared with the observed Bouguer gravity anomaly (black dashed line).
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V.K. Pedersen et al. / Earth and Planetary Science Letters 446 (2016) 1–9
lithosphere and flexural effects that are not related to the local
crust. We therefore constrain our reference crustal model by testing our approach for different reference Moho depths against the
observed gravity anomaly below the high topography in southern Norway (Fig. 2B). The observed Gravity anomalies are available from BGI (http://bgi.omp.obs-mip.fr/); computed from the
EGM2008 spherical harmonic coefficients (Pavlis et al., 2012) and
topography- and Bouguer-corrected (Fuella et al., 2008). Model
gravity anomalies are calculated using a spectral approach (Blakely,
1996). We find the best fit to the gravity anomaly with a reference
Moho depth of ∼33 km (Fig. 3), whereas a reference Moho depth
of either 30 km (Fig. S1A) or 35 km (Fig. S1B) leads to a predicted
gravity anomaly below the high topography in southern Norway
that is either too large or too small.
2.2. Correction of lower-crust velocities
Beyond southern Norway we increase lower-crustal velocities
and corresponding densities when the estimated isostatically compensated topography is significantly higher than the observed topography (Fig. 3B, Fig. S2). Such a correction is required because
our velocity model is constrained only by refraction seismic studies from southern Norway (Stratford et al., 2009). The correction
is done by increasing the two lowermost tie-point velocities cellwise in an iterative manner until predicted isostatic topography
for the given cell or one of its neighboring cells is within a threshold of 50 m from the true topography (Fig. 3B). We find that this
approach and choice of topographic threshold yields a good fit
between observed and modeled gravity anomalies (Fig. 3C). This
increase is also in accord with previous studies that proposed highvelocity, high-density lower crust in the thick, cold Baltic shield
(Ebbing, 2007; Ebbing et al., 2012; England and Ebbing, 2012).
Moreover, offshore seismic observations and gravity modeling suggest that a high-velocity lower crustal body of partially
eclogitized material is located at the coast of southern Norway
(Christiansson et al., 2000). This implies that offshore and along
the western coast of Norway, the seismically observed Moho does
not correspond to the base of the crust, but rather to a change
in velocity from ‘normal’ crust to a high-velocity lower crustal
body. In order to match these seismic offshore observations and
the gravity anomaly along the coastline (Fig. 3B–C), we include a
high-density lower crustal body along the west coast of southern
Norway from the seismically defined Moho down to a depth of
35 km (Fig. 3B, Fig. S3).
2.3. Regional isostatic compensation of topography
We also consider the effects of the lithosphere having a finite
strength, by comparing the deflections that occur when loading a
thin elastic plate with the positive load of the topography (mass
excess) and the negative load of the crustal root (equivalent to a
mass deficit at the surface), respectively (Fig. S5). We note that
the topographic load will be negative in regions where fjord erosion has over-deepened the landscape. Because our crustal density model includes lateral variations we find this negative load
of the mass deficit by first integrating the load of the entire
crustal column and then subtracting the load of the corresponding reference column. In order to incorporate spatial variations in
lithospheric strength (Fig. 1b), we adopt an Alternating-DirectionImplicit technique to solve for the flexural isostatic response of a
given load (Pelletier, 2004). Model parameters used are Young’s
modulus (70 GPa) and Poisson’s ratio (0.25). Herein we adopt
the effective elastic thickness determined from Bouguer coherence
analysis of northern Europe by Pérez-Gussinyé and Watt (2005).
The ratio between plate deflections resulting from the positive
load of the topography and the negative load of the mass deficit at
depth (Supplementary Fig. S5) will give a measure of the degree of
regional compensation, pctcompensated :
pctcompensated =
w root
w topo
· 100%
where w topo is the deflection due to topography and w root is the
deflection due to the mass deficit at depth acting as a crustal root.
Non-compensated topography, on the other hand, is given by
pctnon-compensated (Fig. 3B):
pctnon-compensated = 1 −
w root
w topo
· 100%
To calculate the regionally compensated topography (Fig. 3A),
pctcompensated is multiplied by the observed topography for onshore
regions whereas in fjord regions it is found by interpolation from
onshore regions. The non-compensated (i.e. residual) topography
is then found as the difference between compensated topography
and the observed topography (Fig. 3C). In regions where negative
topography is predicted, we account for water loading as described
above in 2.1.
2.4. Uncertainties in isostatic compensation of topography
Our calculations of isostatic compensation are based on estimates of crustal thickness that include inherent uncertainties
(Stratford et al., 2009) as well as assumptions on: (i) reference
crust, (ii) the extent and density of the high-velocity lower crustal
body at the coastline (Christiansson et al., 2000), and (iii) the velocity structure beyond southern Norway where constraints from
seismic refractions are limited (Stratford et al., 2009). Moreover, we
have omitted possible contributions to isostasy from lateral density heterogeneity within the lithospheric mantle (Gradmann et al.,
2013). Although constrained by observations of gravity, our threedimensional density model is therefore inherently non-unique, especially due to the intrinsic trade-off between crustal density and
thickness, and difficulties distinguishing buoyancy sources from the
crust with those arising from the lithospheric mantle. We stress
in this context that the relatively short wavelength of the gravity
anomaly located under the high topography in southern Norway
points to a buoyancy source in the crust.
Importantly, any combination of subsurface density structure
and Moho thickness that satisfy the observed gravity anomaly
should produce a similar degree of topographic compensation. As
a consequence, the degree of isostatic compensation of topography
we infer in this study should not change significantly as a result of
additional future constraints on the subsurface density structure or
by attributing part of the gravity signal from local buoyancy features in the lithospheric mantle.
2.5. Dynamic topography
Dynamic topography is defined as topography supported by vertical stresses due to viscous flow in the mantle (e.g. Braun, 2010).
Herein, mantle flow and resulting dynamic topography is driven
by density perturbations in the mantle, derived from joint inversions of global seismic and geodynamic data sets, including mineral physical constraints on the conversion of seismic velocities to
densities (Simmons et al., 2007, 2009). A radially symmetric viscosity, inferred from joint inversions of global convection-related
observables and glacial isostatic adjustment data, governs mantle
flow (Mitrovica and Forte, 2004).
In order to include a measure of uncertainty related to this
modeling, we include results from four different models, exploring two different density perturbation models (TX2007 vs. TX2008;
Simmons et al., 2007, 2009) and two different depth-dependent
V.K. Pedersen et al. / Earth and Planetary Science Letters 446 (2016) 1–9
effective viscosity profiles (V1 vs. V2; Forte et al., 2010). Both density models fit global seismic and geodynamic data sets equally
well and differences between the two models arise only from the
inversion parameters used (Simmons et al., 2007, 2009). The two
viscosity profiles also fit observations equally (Forte et al., 2010),
with the greatest difference between V1 and V2 being a low viscosity notch in V1 between the upper and lower mantle (Forte et
al., 2010). Results shown in the main text (Fig. 4D, 5) are based on
the V1 viscosity model (Forte et al., 2010) and the TX2007 density
model (Simmons et al., 2007). Additional models are evaluated in
Supplementary Figs. S6–S8.
Predictions of absolute dynamic topography are highly influenced by the lithospheric mantle, which is often poorly constrained in terms of age, depletion/composition, and/or temperature. The convective models used in this study do include mineral
physical constraints, and compositional effects are taken into account to some degree (Simmons et al., 2007, 2009). However, the
use of a global seismic framework in the inversions is a limiting
factor to the extent in which one may resolve regional lithospheric
mantle heterogeneity. Therefore, we cannot expect the models
to capture regional mantle lithosphere structures specific to the
Scandinavian region (e.g. Gradmann et al., 2013; Maupin, 2011;
Medhus et al., 2012; Rickers et al., 2013). We can ascertain that
there is consensus between global and regional models at depth
(below the lithosphere), however, for the lithospheric mantle this
is not the case. For this reason, we remove contributions to dynamic topography from the upper 200 km, by assuming it neutrally
buoyant (Fig. S6A–D). By doing so, we eliminate any contributions from the poorly constrained (global) lithospheric mantle to
dynamic topography, and as a result get much more consistent predictions from the different model runs (Fig. S6E–H).
Regional studies suggest, however, that the uppermost mantle
in the Scandinavian region may be positively buoyant (Gradmann
et al., 2013; Maupin, 2011; Medhus et al., 2012; Rickers et al.,
2013) compared to the reference density model used in the convection models (PREM; Dziewonski and Anderson, 1981). Such
buoyancy, not captured by our global modeling approach, should
result in negative dynamic topography predictions in southwestern
Scandinavian when assuming the upper 200 km neutrally buoyant (Fig. S6). As an example, a density anomaly of ∼15 kg/m3 will
result in ∼500 m of topography if distributed within the upper
100 km, whereas a density anomaly of <10 kg/m3 will result in
∼500 m of topography if distributed within the upper 200 km.
These values are well within realistic density variations found in
sub-continental lithospheric mantle (Djomani et al., 2001), and
are consistent with expected values found for the Phanerozoic
and Proterozoic mantle lithosphere below the Scandinavian region
(Gradmann et al., 2013), compared to the reference density model
(PREM; Dziewonski and Anderson, 1981).
The regional studies suggest also that there is a significant
difference in the mantle lithosphere found below Norway and
Sweden, respectively, owing to local variations in age, depletion,
thickness, and temperature (Gradmann et al., 2013; Maupin, 2011;
Medhus et al., 2012; Rickers et al., 2013). The mantle lithosphere
below Sweden has been found to be thicker and colder than below
Norway, but is also more depleted. A number of seismic tomography studies also predict low velocities immediately below the
lithosphere in southern Norway, suggesting the presence of hot asthenosphere in this region (Maupin, 2011; Legendre et al., 2012;
Medhus et al., 2012; Rickers et al., 2013). These lateral variations
in temperature and composition may result in variable buoyancy
from within the upper 200 km across the southwestern Scandinavian region, making absolute values of dynamic topography difficult to interpret even when removing contributions from the upper
200 km.
5
We therefore evaluate in the following only changes in dynamic
topography over time (latest 10 Myr) using a backward-in-time
convection scheme and taking into account tectonic plate motion
(Moucha et al., 2008; Moucha and Forte, 2011). By considering
changes in dynamic topography over time, we avoid uncertainties
related to the lithospheric mantle, both in terms of constraining
absolute buoyancy contribution, and in terms of understanding
spatial variability within the region.
3. Results and discussion
In agreement with previous studies (Ebbing and Olesen, 2005;
Ebbing, 2007; Ebbing et al., 2012; Maupin et al., 2013; Stratford
et al., 2009; Stratford and Thybo, 2011), our isostatic calculations
demonstrate that much of the current high topography in western Scandinavia can be explained by the crustal structure (Fig. 4A).
This suggests that significant, more than 1000 m high topography has existed in the region since the formation of the current
crustal structure. In contrast, the western-most part of southern
Norway shows negative predictions of isostatically compensated
topography (Fig. 4A) and indicates that the current topography in
this area is poorly explained by crustal structure. Consequently, the
residual topography ranges locally from fully compensated in the
high-elevated areas in central southern Norway to completely uncompensated (+1000 m) along the west coast (Fig. 4C). Much of
this local variability may be ascribed to lithology, rock strength,
and differential erosion, and most regions show less extreme values, with a general trend of decreasing isostatic compensation toward the west coast (Fig. 4B). On average ∼300 m of topography
is uncompensated by the current crustal structure in southwestern
Norway.
Accordingly, a mechanism unrelated to crustal structure is
needed in order to explain the uncompensated residual topography found in southwestern Norway (∼300 m), and observed
low velocities in the upper mantle may suggest a dynamic origin related to mantle flow (Maupin, 2011; Medhus et al., 2012;
Rickers et al., 2013). A sub-lithospheric origin linked to convection
could also explain the generally positive free-air gravity anomaly
in this part of the region (Fig. 2C; Molnar et al., 2015).
Spatial patterns in dynamic topography change in Scandinavia
over the last 10 Myr are remarkably consistent between the different evaluated models, showing positive values in southern Norway
and close to zero or negative values in the rest of the region
(Fig. 4D, Fig. S7). This is in agreement with previous work from
the broader region (Steinberger et al., 2015; Marquart and Schmeling, 2004) and suggests dynamic surface uplift for southwestern
Norway within the last 10 Myr, with an increasing trend toward
the coast, and concurrent dynamic subsidence that increases toward the east (Fig. 4D, Fig. S7).
As illustrated by the variability in amplitudes between the
models, absolute values of dynamic topography are difficult to assess, as minor uniform regional changes in density may shift absolute values without significantly degrading the global fit to the
models’ geodynamic constraints (Fig. S7; Forte et al., 2010). Long
wavelength spatial gradients in dynamic topography are, however,
more robust as they arise from the large-scale flow field that
is consistent with the long wavelength geodynamic constraints.
We find consistently for all evaluated models an uplift gradient
of ∼200–300 m from east to west in southwestern Scandinavia
(Fig. 4D, Fig. S7). These dynamic surface motions are predicted as
a consequence of passive upwelling below the southern margin of
Norway that is part of a larger convective cell as shown in the regional cross-sections (Fig. 5, Fig. S8).
The strong correlation in both spatial distribution and amplitude between isostatic residual topography (Fig. 4B–C) and recent
changes in dynamic topography (Fig. 4D) suggests local rejuvena-
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V.K. Pedersen et al. / Earth and Planetary Science Letters 446 (2016) 1–9
Fig. 4. Regional isostatic, residual, and dynamic topography. A. Topography compensated by the crust. Regions with negative predicted topography have been corrected
for water load. B. Degree of topography not compensated by the crust. Contour lines represent 50% and 100% non-compensation. C. Residual topography (real topography
minus isostatically compensated topography from A). Positive values represent regions where the present topography is higher than expected from the crustal structure, and
negative values regions where the topography is lower than expected. D. Dynamic topography change since 10 Ma (TX2007V1; Simmons et al., 2007; Forte et al., 2010).
Positive values indicate rock uplift whereas negative values correspond to subsidence. Black dashed line represents the profile shown in Fig. 2.
V.K. Pedersen et al. / Earth and Planetary Science Letters 446 (2016) 1–9
7
Fig. 5. Mantle temperature structure and flow. A. Present-day thermal structure derived from the TX2007 density model (Simmons et al., 2007), with mantle flow calculated
for the V1 viscosity model (Forte et al., 2010). The cross-section coincides with the cross-section shown in Figs. 2–4 of the main text, with the points at the surface marking
the west coast of Norway (4.6E, 60.5N) and east coast of Sweden (17.0E, 60.9N), respectively. B. Corresponding backwards advected mantle temperatures and mantle flow at
10 Ma. The green in lines across the sections are depth markers at: 410 km, 660 km, and 2000 km. The base of the figure represents the core–mantle boundary (CMB).
tion of already existing topography in southwestern Norway during
the last 10 Myr. The uplift is mostly prevalent near the coastal
regions and decreases inland toward the highest topography that
appears to be largely compensated by the crustal structure.
In this study we have not considered explicitly buoyancycontributions from the lithospheric mantle. However, lateral variations in density owing to a spatially varying lithospheric thickness
may contribute to compensate the present topography. Indeed, following previous work by Gradmann et al. (2013), a lithospheric
thinning of ∼30 km across southern Norway could account for
some (∼100–200 m) of the inferred residual topography (Fig. 4C),
if a density contrast of ∼10–20 kg/m3 is assumed across the
lithosphere–asthenosphere boundary (LAB), as suggested by geodynamic modeling in the region (Gradmann et al., 2013). Such
minor long-wavelength features may not be captured in the gravity anomaly map and resolved by the gravity modeling approach
used, and should therefore be considered in addition to the isostatic compensation found in this study. More significant buoyancy
contributions from within the lithospheric mantle should be recognizable from the gravity anomaly, and such contributions are
therefore already accounted for in our approach (see section 2.4).
Topography compensated by a density contrast across the LAB
for a spatially varying lithosphere thickness could be related to
the original lithospheric architecture in the region or to erosion at
the base of the lithosphere by small-scale mantle convection. We
note in this context that our inferred residual topography (Fig. 4C)
shows an increasing trend toward the North Sea basin and not the
current spreading axis in the north Atlantic. This may suggest that
any base-lithosphere erosion was related to rifting in the North
Sea in Mesozoic times (e.g. Glennie, 1998), as opposed to more recent Cenozoic events in the north Atlantic. Therefore, we do not
rule out that buoyancy contributions from the lithospheric mantle
may contribute to the present topography. However, we suspect
that such contributions predate recent (<10 Ma) dynamic surface
uplift inferred in this study.
Our results provide strong support for an old Caledonian age of
most high topography in western Scandinavia, given that the most
recent crustal thickening occurred during the Caledonian orogeny.
However, a component of the topography along the west coast of
southern Norway is found not to be in isostatic equilibrium. Although of moderate amplitude (in average ∼300 m), this result is
well constrained by the observed gravity anomaly in southwestern
Scandinavia, and it is therefore a robust outcome, regardless of the
uncertainly associated with the crustal model in use.
By suggesting significant isostatic support of the high mountains in southern Norway, in combination with recent modest
dynamic topographic rejuvenation of the coastal area, our hypothesis includes components from both previous hypotheses for
long-term topographic evolution in western Scandinavia (Fig. 1,
Hypothesis 3). Although of amplitude much smaller than previously suggested by the peneplain hypothesis (Fig. 1, Hypothesis 1),
recent dynamic uplift of the coastal areas in southern Norway
provides an additional mechanism of uplift to the isostatic rockcolumn uplift expected as a consequence of erosional unloading.
This modest topographic rejuvenation is, in combination with a
general eustatic sea-level fall (Miller et al., 2005) and concurrent
erosion-driven isostatic rock-column uplift, consistent with observations of increased sedimentation since ∼10 Ma, over-burial of
coast-proximal tilted sedimentary strata, and an angular unconformity at the base of the Quaternary (e.g. Japsen, 1988; Riis, 1996;
Stuevold and Eldholm, 1996). As previously suggested by Nielsen et
al. (2009), these offshore observation may be explained by climatedependent erosion-driven rock-column uplift in the onshore and
offshore subsidence due to sediment loading, in combination with
recent glacial reworking of shelf sediments. However, from the
study presented here, we have good reason to believe that some
part of the offshore signal is due to a modest dynamic uplift of
the coastal region, and the exposure and reworking of shelf sediments that this would have facilitated.
Our results show that high-elevation low-relief regions in western Scandinavia cannot represent a dissected Mesozoic peneplain
uplifted in Neogene times. Recent peneplain uplift is simply incompatible with the large degree of isostatic support of topography
we find in this study. We suggest that low-relief regions in western
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Scandinavia represent a generally low-relief landscape (a remnant
of Caledonian topography) that has experienced glacial erosion at
high elevation (Pedersen and Egholm, 2013; Steer et al., 2012) and
been smoothened by altitudinal-dependent periglacial processes
(Anderson, 2002; Egholm et al., 2015). The low relief landscape has
been dissected by fluvial and glacial activity – processes that have
been amplified by (i) a general eustatic sea level fall since the Cretaceous (Miller et al., 2005), (ii) modest dynamic uplift since the
Neogene owing to mantle convection (∼300 m), and last but not
least (iii) climate cooling leading to substantial isostatic uplift resulting from unloading by differential glacial erosion.
4. Conclusions
Globally, the origin of elevated rifted passive continental margins is enigmatic and highly debated with a range of competing
hypotheses. By quantifying contributions from crustal isostasy and
dynamic topography in southwestern Scandinavia we constrain
age, origin, and recent evolution of topography in this region. By
providing a quantitative explanation that combines elements from
pre-existing end-member hypotheses, the results presented here
provide a new perspective on the long-standing controversy on the
origin of high passive-margin topography in Scandinavia. Remnant
topography from the Caledonian orogeny, modified by North Atlantic rifting and influenced by recent dynamic surface motions,
control present-day topography along this continental margin.
Based on our results we reject the century-old idea of an uplifted, dissected peneplain existing in western Scandinavia. Recent
peneplain uplift is simply incompatible with the large degree of
isostatic support of topography we find in this study.
Acknowledgements
We thank M. Pérez-Gussinyé for providing the effective elastic
thickness map and S. Gac for providing the code used for gravity
calculations. V.K.P. acknowledges financial support from the Research Council of Norway under the FRINATEK program. We thank
two anonymous reviewers for thorough and constructive comments.
Appendix A. Supplementary material
Supplementary material related to this article can be found online at http://dx.doi.org/10.1016/j.epsl.2016.04.019.
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